A Course in Theoretical Physics
eBook - ePub

A Course in Theoretical Physics

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eBook - ePub

A Course in Theoretical Physics

About this book

This book is a comprehensive account of five extended modules covering the key branches of twentieth-century theoretical physics, taught by the author over a period of three decades to students on bachelor and master university degree courses in both physics and theoretical physics.

The modules cover nonrelativistic quantum mechanics, thermal and statistical physics, many-body theory, classical field theory (including special relativity and electromagnetism), and, finally, relativistic quantum mechanics and gauge theories of quark and lepton interactions, all presented in a single, self-contained volume.

In a number of universities, much of the material covered (for example, on Einstein's general theory of relativity, on the BCS theory of superconductivity, and on the Standard Model, including the theory underlying the prediction of the Higgs boson) is taught in postgraduate courses to beginning PhD students.

A distinctive feature of the book is that full, step-by-step mathematical proofs of all essential results are given, enabling a student who has completed a high-school mathematics course and the first year of a university physics degree course to understand and appreciate the derivations of very many of the most important results of twentieth-century theoretical physics.

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Information

Edition
1
Subtopic
Physics
Index
Physics
Module III
Many-Body Theory
13
Quantum Mechanics and Low–Temperature Thermodynamics of Many–Particle Systems
13.1 Introduction
By a “many–particle system” we shall mean a system of macroscopic size (for example, one for which the number of particles is of the order of 1023).
By “low–temperature” we shall mean that the temperature T is such that (a) the system is only weakly excited relative to the ground state and (b) quantum statistics is necessary (Fermi–Dirac for fermions, Bose–Einstein for bosons), that is, the quantum–mechanical principle of indistinguishability of identical particles has macroscopic consequences. (An example of the latter is the dramatic difference in the properties of liquid helium–3 and liquid helium–4.)
The properties to be studied in this chapter include:
(a) the wave function and energy of the ground state of the system;
(b) the wave functions, energies and widths (inverse lifetimes) of weakly excited states;
(c) the thermodynamic state variables [found from the energies from (b) by the methods of statistical mechanics].
13.2 Systems of noninteracting particles
The hamiltonian
inline
of a system of noninteracting particles can be written as:
(13.1)
Equation
where
inline
n is the hamiltonian of particle n, and
inline
clearly contains no potential energies of interaction of the type
inline
nm.
The single–particle energy eigenstates (eigenstates of
inline
n) may be written as
(13.2)
Equation
with corresponding energy eigenvalues Δαi:
(13.3)
Equation
The symbol α denotes the set of quantum numbers corresponding to a complete set of single–particle observables. For example, for an electron moving in the Coulomb potential of a nucleus the set α could be the set n,l,m,ms (see section 1.17 on hydrogenic states), while for a free particle with spin the set α could be the set kx, ky, kz, ms. The different sets of possible numerical values of the quantum numbers in a given set α are labelled by the index i, which may be considered to take integer values from 1 to ∞, using any chosen ordering convention. For example, we could choose i = 1 to correspond to the set of quantum-number values for the ground state of the part...

Table of contents

  1. Cover
  2. Title Page
  3. Copyright
  4. Dedication
  5. Notation
  6. Preface
  7. Module I: Nonrelativistic Quantum Mechanics
  8. Module II: Thermal and Statistical Physics
  9. Module III: Many-Body Theory
  10. Module IV: Classical Field Theory and Relativity
  11. Module V: Relativistic Quantum Mechanics and Gauge Theories
  12. Appendices
  13. Supplementary Reading
  14. Index

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